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Classification of Chandra X-Ray Sources in Cygnus OB2

We have devised a predominantly Naive Bayes−based method to classify X-ray sources detected by Chandra in the Cygnus OB2 association into members, foreground objects, and background objects. We employ a variety of X-ray, optical, and infrared characteristics to construct likelihoods using training s...

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Salvato in:
Autori principali: Vinay L. Kashyap, Mario G. Guarcello, Nicholas J. Wright, Jeremy J. Drake, Ettore Flaccomio, Tom L. Aldcroft, Juan F. Albacete Colombo, Kevin Briggs, Francesco Damiani, Janet E. Drew, Eduardo L. Martin, Giusi Micela, Tim Naylor, Salvatore Sciortino
Natura: Artigo
Lingua:Inglês
Pubblicazione: IOP Publishing 2023-01-01
Serie:The Astrophysical Journal Supplement Series
Soggetti:
Star forming regions
Catalogs
Astrostatistics
Astrostatistics techniques
Bayesian statistics
Open star clusters
Accesso online:https://doi.org/10.3847/1538-4365/acdd68
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